Report on the Radiolaria Collected by H.M.S. Challenger During the Years 1873-1876, First Part: Porulosa (Spumellaria and Acantharia): Report on the Scientific Results of the Voyage of H.M.S. Challenger During the Years 1873-76, Vol. XVIIIHaeckel, Ernst
Science
Report on the Radiolaria Collected by H.M.S. Challenger During the Years 1873-1876, First Part: Porulosa (Spumellaria and Acantharia): Report on the Scientific Results of the Voyage of H.M.S. Challenger During the Years 1873-76, Vol. XVIII
Haeckel, Ernst
Radiolaria
245. _Abundance of Radiolaria in the Various Rocks._--The relative quantity
of well-preserved or at all events recognisable Radiolaria in the different
rocks is very variable. In this respect three different degrees may be
distinguished, which may be called shortly "pure, mixed, and poor"
Radiolarian formations. The _pure_ Radiolarian rocks consist for the
greater part (usually much more than half, sometimes even more than
three-quarters) of closely compacted often calcined masses of siliceous
Polycystine shells. To this category belong the pure Miocene Polycystine
marls of Barbados (§ 246), the Tertiary Polycystine clay of the Nicobar
Islands (§ 247), and the Polycystine quartz of the Jura (§ 248). All these
pure Radiolarian rocks may be regarded as fossil Radiolarian ooze (§ 237),
and are certainly of deep-sea origin, having probably been deposited at
depths greater than 2000 fathoms. Their palæontological character also is
in favour of this view, for the abyssal Osculosa (§ 235) are more abundant
and richer in species than the pelagic Porulosa (§ 233). The elevation of
this deep-sea layer above the surface of the sea appears to have taken
place but seldom; it has only been observed on a large scale at Barbados
and in the Nicobar Islands. The _mixed_ Radiolarian rocks are much more
common; they were probably deposited at much less depths, or perhaps are
not true deep-sea formations at all. The siliceous shells of Polycystina
always constitute less than half (sometimes less than one-tenth) of their
mass, and are less prominent than other siliceous remains (Diatoms), or
calcareous remains (Foraminifera), or in some cases than the mineral
constituents (pumice, &c.). To this group belong many of the
above-mentioned Tertiary marls and clays (especially the Mediterranean
Tripoli), also many flints, cherts, and other quartzites from Mesozoic
strata (especially from the Jura), and probably also some palæozoic
quartzites. The marine ooze from which they have originated may have been
deposited at very various, even at slight, depths of the ocean. Formations
_poor_ in Radiolaria, which contain only a few species of SPUMELLARIA and
NASSELLARIA mingled with other fossil remains and mineral particles, occur
in all formations and are probably very widely distributed. Further careful
examination of thin sections (especially of coprolites) will yield here a
rich harvest of new forms. Both the mixed and the pure Radiolarian
formations may be divided according to their petrographic characters into
three groups, which, however, are connected by intermediate varieties--(1)
soft, chalky marl (§ 246), (2) plastic clay (§ 247), and (3) hard, flinty
quartz (§ 248).
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